Theta Herculis
Historical view of the Hercules constellation showing Rukbalgethi Genubi (θ Her) as the "southern knee", right of center | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hercules |
| Right ascension | 17h 56m 15.18054s |
| Declination | +37° 15′ 01.9343″ |
| Apparent magnitude (V) | 3.851 |
| Characteristics | |
| Spectral type | K1IIaCN2 |
| U−B color index | +1.40 |
| B−V color index | +1.35 |
| R−I color index | +0.63 |
| Variable type | Irregular (suspected) |
| Astrometry | |
| Radial velocity (Rv) | –28.32 km/s |
| Proper motion (μ) | RA: 2.67 mas/yr Dec.: 6.47 mas/yr |
| Parallax (π) | 4.33±0.13 mas |
| Distance | 750 ± 20 ly (231 ± 7 pc) |
| Absolute magnitude (MV) | −2.71+0.26 −0.23 |
| Details | |
| Mass | 5.89±0.07 M☉ |
| Radius | 82±2 R☉ |
| Luminosity | 2,410±150 L☉ |
| Surface gravity (log g) | 1.37±0.04 cgs |
| Temperature | 4,448±23 K |
| Metallicity [Fe/H] | −0.03±0.15 dex |
| Rotational velocity (v sin i) | 3.4 ± 0.6 km/s |
| Age | 130 Myr |
| Other designations | |
| Rukbalgethi Genubi, θ Her, 91 Her, BD+37°2982, FK5 672, GC 24415, HD 163770, HIP 87808, HR 6695, SAO 66485 | |
| Database references | |
| SIMBAD | data |
Theta Herculis is a single, variable star in the northern constellation of Hercules. This object is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 3.851. Based upon parallax measurements, it is located around 750 light years away from the Sun. The star is advancing toward the Earth with a heliocentric radial velocity of –28 km/s.
This is an aging K-type bright giant with a stellar classification of K1IIaCN2, where the suffix notation indicates a strong overabundance of CN in the spectrum. The brightness variations of this star was first noticed in 1935 by M. Fedtke and confirmed by Erich Przybyllok and Kurt Walter the same year. French astronomer Paul Muller then classified Theta Herculis as an irregular variable with a range of magnitudes between 3.7 and 4.1 and a periodicity of roughly 8–9 days.
The star is about 130 million years old with 5.89 times the mass of the Sun. With the hydrogen at its core exhausted, the star has expanded to 82 times the Sun's radius. It is radiating 2,400 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,448 K.